Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems
Abstract
Continuous gravitational waves, i.e., persistent and nearly-monochromatic signals emitted by asymmetric spinning neutron stars, remain elusive. Searches for these signals from unknown binary systems are the most computationally challenging, but they are essential, given that binary accretion provides a natural mechanism for creating the required asymmetry, and around half of the known pulsars rotating above 25 Hz are part of a binary system. Here we report on a search of a large uncharted parameter-space region: for the first time we cover gravitational-wave frequencies above 520 Hz (from 50 to 1000 Hz), and, for the first time with advanced detectors, orbital periods lower than 3 days are explored. No signal is detected, and we set the most stringent constraints to date on the amplitude of signals of this kind. Our results exclude with 95% confidence neutron stars within 100 pc and rotating faster than ∼ 495 Hz from having ellipticities above 5.2 × 10−8. Within the same distance our results also exclude r-mode amplitudes above 1.5 × 10−6 for stars rotating faster than ∼ 740 Hz.
Versions
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BibTeX
@misc{covas2026wide,
title = {{Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems}},
author = {P. B. Covas and M. A. Papa and R. Prix},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2605.14728},
eprint = {2605.14728},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2605.14728},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems
AU - P. B. Covas
AU - M. A. Papa
AU - R. Prix
PY - 2026
DA - 2026/09/18
PB - arXiv
DO - 10.48550/arxiv.2605.14728
UR - https://arxiv.org/abs/2605.14728
AB - Continuous gravitational waves, i.e., persistent and nearly-monochromatic signals emitted by asymmetric spinning neutron stars, remain elusive. Searches for these signals from unknown binary systems are the most computationally challenging, but they are essential, given that binary accretion provides a natural mechanism for creating the required asymmetry, and around half of the known pulsars rotating above 25 Hz are part of a binary system. Here we report on a search of a large uncharted parameter-space region: for the first time we cover gravitational-wave frequencies above 520 Hz (from 50 to 1000 Hz), and, for the first time with advanced detectors, orbital periods lower than 3 days are explored. No signal is detected, and we set the most stringent constraints to date on the amplitude of signals of this kind. Our results exclude with 95% confidence neutron stars within 100 pc and rotating faster than ∼ 495 Hz from having ellipticities above 5.2 × 10^−8. Within the same distance our results also exclude r-mode amplitudes above 1.5 × 10^−6 for stars rotating faster than ∼ 740 Hz.
ER -